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1) AIM/CIPS noctilucent cloud images and movies, etc. maxmize
Resource ID:spase://VSPO/NumericalData/AIM/CIPS/PT90M
Start:2007-06-01 00:00:00 Observatory:AIM Cadence:90 minutes
Stop:2016-09-14 08:00:04 Instrument:AIM Cloud Imaging and Particle Size experiment Resource:NumericalData
AIM/CIPS (Cloud Imaging and Particle Size) data are available in multiple processing levels: 1a (calibrated and geolocated albedo); 1b (map- projected albedo at 5km x 5km resolution); 1c (same as 1b, but with Rayleigh scattering background subtracted); 2 (imagery for 15 orbit- specific strips per day, built from 1c data); 3a (daily "daisies" built as composites over level 2 data); 3b (seasonal movies built from level 3a data); 4 (cloud properties such as ice water content and particle radius extracted from lower level data). Data files for levels 2, 3a and 4 are accessible from http://aim.hamptonu.edu/sds/cal_index_aim.php?instrument=cips, with level 2 and 4 data as gzipped netCDF's and level 3a imagery in PNG format. Brief descriptions of data levels, browse imagery, and links to fuller data documentation files at LASP are available from http://aim.hamptonu.edu/library/documentation/instruments/cips/cips_docs.html Data are available over each polar region about 4 months each year, during that region's summer.(

2) Akebono ATV auroral images maxmize
Resource ID:spase://VSPO/DisplayData/Akebono/ATV/PT3H
Start:1989-04-12 00:00:00 Observatory:Akebono Cadence:3 hours
Stop:1990-02-28 00:00:00 Instrument:Akebono Auroral TV Imagery(ATV) Resource:NumericalData
These Akebono ATV auroral images are available at somewhat irregular time intervals. There are also a few brief movies of various types of auroral forms.

3) Solar Data at Meudon and Tarbes via BASS 2000 maxmize
Resource ID:spase://VSPO/NumericalData/BASS2000/SolarData
Start:1989-12-01 00:00:00 Observatory:Meudon Cadence:
Stop:2016-09-14 07:59:52 Instrument:Meudon Spectroheliograph Resource:NumericalData
Multiple solar data products held at Meudon and Tarbes sites in France, via the BASS (Base de donnees Solaire Sol) 2000 web site. Included are Nancay radioheliograph data, Meudon spectroheliograph data, THEMIS data and Pic du Mida coronagraph data

4) SMEI Imagery of CME's maxmize
Resource ID:spase://VSPO/DisplayData/Coriolis/SMEI/IMAGES
Start:2003-03-31 00:00:00 Observatory:Coriolis Cadence:
Stop:2016-09-14 07:59:48 Instrument:Solar Mass Ejection Imager (SMEI) Resource:DisplayData
Images and movies from the Solar Mass Ejection Imager (SMEI) flown on the USAF Coriolis spacecraft

5) DE 1 Spin-Scan Auroral Imager UV Images maxmize
Resource ID:spase://VSPO/NumericalData/DE1/SAI/PT3M
Start:1981-09-23 00:00:00 Observatory:Dynamics Explorer 1 Cadence:3 minutes
Stop:1991-02-18 00:00:00 Instrument:DE 1 Spin-Scan Auroral Imager Resource:NumericalData
This data set contains ultraviolet images in quasi-logarithmically compressed counts from the vacuum ultraviolet imaging photometer of the Spin-Scan Auroral Imager (SAI) flown on DE 1. The time resolution was 3 to 12 minutes per image. Also included are the GCI position vector, velocity vector and spin axis of the spacecraft. Data are available in CDF format from CDAWeb.

6) Evans Solar Facility Spectroheliographs maxmize
Resource ID:spase://VSPO/NumericalData/EvansSolarFacility/Spectroheliograph/PT86400S
Start:1996-02-05 00:00:00 Observatory:Evans Solar Facility Cadence:86400 seconds
Stop:1999-05-28 00:00:00 Instrument:Evans Solar Facility (ESF) Spectroheliograph Resource:NumericalData
Daily Solar Full Disk Spectroheliographs at 6563A and 3934A taken at John W. Evans Solar Facility

7) GOES SXI Solar X-Ray Images maxmize
Resource ID:spase://VSPO/NumericalData/GOES/12/SXI/PT60.00S
Start:2001-08-16 00:00:00 Observatory:GOES 12 Cadence:60.00 seconds
Stop:2016-09-14 08:00:05 Instrument:GOES 12 Solar X-Ray Imager Resource:NumericalData
GOES SXI Solar X-Ray Images in FITS format

8) Mauna Loa Solar Observatory ACOS/CHIP LOS_Velocity Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/CHIP/LOS-Velocity.Images
Start:1996-04-20 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar line-of-sight velocity images (dopplergrams) and movies from the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm) of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'chp' rather than 'CHIP'.

9) Mauna Loa Solar Observatory ACOS/CHIP Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/CHIP/Solar.Images
Start:1996-04-20 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar images and movies from the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm) of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'chp' rather than 'CHIP'.

10) Mauna Loa Solar Observatory ACOS/MK4 Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/MK4/Solar.Images
Start:1998-10-01 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar coronal images and movies in white light polarization brightness from the Mark-IV (Mk4) instrument of the Advanced Coronal Observing System (ACOS)

11) Mauna Loa Solar Observatory PICS and DPM Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/PICS-DPM/Solar.Images
Start:1994-02-02 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) H-alpha solar disk and limb images and movies from the Polarimeter for Inner Coronal Studies (PICS) and the Digital Prominence Monitor (DPM) that PICS replaced in September, 1997. PICS is part of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'dpm' for both DPM and PICS.

12) Solar Imagery from Mauna Loa Solar Observatory at HAO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/Solar.Images
Start:1980-01-01 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar images and movies from the Advanced Coronal Observing System (ACOS), the Experiment for Coordinated Helioseismic Observations (ECHO) and the Precision Solar Photometric Telescope (PSPT). ACOS includes the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm), H-alpha prominence and solar disk monitor (PICS, 656.2 nm), and the Mk4 K-coronameter (sees white light K-corona from 1.12 to 2.79 solar radii). ECHO observes oscillations in solar surface radial velocities. PSPT observes the solar disk in three bandpasses: 605-610 nm (red), 408-412 nm (blue) and 393 nm (Ca II K). Some MLSO data contribute to the GONG program.

13) Hinode data (all-inclusive) via Project Page or DARTS maxmize
Resource ID:spase://VSPO/NumericalData/Hinode/PT1M
Start:2006-10-01 00:00:00 Observatory:Hinode Cadence:1 minute
Stop:2016-09-14 08:00:04 Instrument:Solar Optical Telescope Resource:NumericalData
A wealth of Hinode movie, image and digital data are accessible via links from the NASA/MSFC Project web page and from the DARTS data archive in Japan. Data are from all three instruments, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT) and the EUV Imaging Spectrometer (EIS)

14) IBEX-Hi Direct Events maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Hi/Direct_Events
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Hi Resource:NumericalData
Each record captures the characteristics of one energetic neutral atom arriving at IBEX-Hi. Included is a time tag (seconds since 00:00 UT of January 6, 1980), an arrival direction (R.A. and Dec. in J2000 celestial coordinates), the IBEX location, ENA energy band and coincidence type. Positive species identifications are not made, but most arriving ENA's are hydrogen atoms. Data files are given for each 8-day orbit and for each of the 6 IBEX-Hi energy bands. The data files are in ASCII.

15) IBEX-Hi Histograms maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Hi/Histograms
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Hi Resource:NumericalData
Each record captures the number of arriving ENA's of a specific energy band, coincidence type, and spin phase. Data for each full ~15s spacecraft spin are given at each of 60 spin phases in sequential records, with the J2000 right ascension and declination for look directions corresponding to each spin phase being given in the corresponding record. Also included in each record are a time tag (seconds since 00:00 UT of January 6, 1980), the IBEX location, ENA energy band and coincidence type. Positive species identifications are not made, but most arriving ENA's are hydrogen atoms. Data files are given for each 8-day orbit and for each of the 6 IBEX-Hi energy bands. The data files are in ASCII.

16) IBEX-Hi maps in PNG display format maxmize
Resource ID:spase://VEPO/DisplayData/IBEX/Hi/Maps-PNG
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 months
Stop:2015-12-14 07:55:37 Instrument:IBEX-Hi Resource:DisplayData
As of this writing (11/5/2010), this product had been issued by the IBEX team in two releases. Release 1 IBEX-Hi map data are superseded by Release 2 data which are more time-extensive (12 months vs. 6 months) and are richer in content. While Release 1 IBEX-Hi map data and their documentation remain accessible at ftp://spdf.gsfc.nasa.gov/pub/data/ibex/hi/maps/digital_data/release_1/ and ftp://spdf.gsfc.nasa.gov/pub/data/ibex/hi/maps/images/release_1/, this description supports the retrieval and use of Release 2 data only. The Release_2 IBEX-Hi map data contain all-sky 6 deg x 6 deg resolution maps in J2000 ecliptic coordinates of energetic neutral fluxes reaching the near-Earth IBEX spacecraft from the distant heliosphere and heliosheath. Maps are in both a spacecraft frame and, via Compton-Getting corrections, a heliospheric frame. Basic maps are each accumulated over 6-months duration, so far for epochs 1 (12/2008-06/2009) and 2 (06/2009-12/2009). Maps are available for five of the energy bands of IBEX-Hi (0.52-0.95, 0.84-1.55, 1.36-2.50, 1.99-3.75, 3.13-6.00 keV) and, for the heliospheric frame only, also for six monoenergetic points (0.71, 1.11, 1.74, 2.73, 3.0, 4.29 keV). In addition, monoenergetic maps are available as summed over the data collected during epochs 1 and 2 combined. All maps are available in digital text format and in PNG image format (considered as separate data sets within VEPO). Given that VHO/VEPO typically displays clickable granule (file) names for any given specification of data product and time span, and given that IBEX-Hi digital maps and PNG-formatted display maps are each considered single data products, a request for data from either product will yield .GE.20 names of files containing data spanning or within the requested time span. For IBEX, the names shown by VHO/VEPO actually have the form subdirectory/filename. The subdirectories are named map1, map1cg, map2, map2cg, and map-combined. Maps involving "1" ("2") are from the first (second) 6-month epoch, while "combined" means composed of data taken during epochs 1 and 2. Maps involving (not involving) "cg" means heliospheric frame (spacecraft frame). In the first four subdirectories, file names are of the forms ha60.hide-trp-flux100-hi-N-flux.ext and ha60.hide-trp-mono_80-P.PP-flux.ext, where "ext" is "png" or "txt" according to which product is requested, N is the energy step number for the IBEX-Hi instrument (2-6), P.PP is the energy level, in keV, of a monoenergetic flux. Files in the "combined" subdirectories are named "combined-P.PP-flux.ext, where P.PP has the same meaning as above. In addition to the flux maps to which VEPO provides access, several map files whose data support the determination of the fluxes are also available in the underlying nssdcftp directories and are described by aareadme files there (and by IBEX web pages at SWRI: http://ibex.swri.edu/ibexpublicdata/Data_Release_2/)

17) IBEX-Hi digital maps every 6 months maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Hi/Maps-TXT
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 months
Stop:2015-12-14 07:55:45 Instrument:IBEX-Hi Resource:NumericalData
As of this writing (11/5/2010), this product had been issued by the IBEX team in two releases. Release 1 IBEX-Hi map data are superseded by Release 2 data which are more time-extensive (12 months vs. 6 months) and are richer in content. While Release 1 IBEX-Hi map data and their documentation remain accessible at ftp://spdf.gsfc.nasa.gov/pub/data/ibex/hi/maps/digital_data/release_1/ and ftp://spdf.gsfc.nasa.gov/pub/data/ibex/hi/maps/images/release_1/, this description supports the retrieval and use of Release 2 data only. The Release_2 IBEX-Hi map data contain all-sky 6 deg x 6 deg resolution maps in J2000 ecliptic coordinates of energetic neutral fluxes reaching the near-Earth IBEX spacecraft from the distant heliosphere and heliosheath. Maps are in both a spacecraft frame and, via Compton-Getting corrections, a heliospheric frame. Basic maps are each accumulated over 6-months duration, so far for epochs 1 (12/2008-06/2009) and 2 (06/2009-12/2009). Maps are available for five of the energy bands of IBEX-Hi (0.52-0.95, 0.84-1.55, 1.36-2.50, 1.99-3.75, 3.13-6.00 keV) and, for the heliospheric frame only, also for six monoenergetic points (0.71, 1.11, 1.74, 2.73, 3.0, 4.29 keV). In addition, monoenergetic maps are available as summed over the data collected during epochs 1 and 2 combined. All maps are available in digital text format and in PNG image format (considered as separate data sets within VEPO). Given that VHO/VEPO typically displays clickable granule (file) names for any given specification of data product and time span, and given that IBEX-Hi digital maps and PNG-formatted display maps are each considered single data products, a request for data from either product will yield .GE.20 names of files containing data spanning or within the requested time span. For IBEX, the names shown by VHO/VEPO actually have the form subdirectory/filename. The subdirectories are named map1, map1cg, map2, map2cg, and map-combined. Maps involving "1" ("2") are from the first (second) 6-month epoch, while "combined" means composed of data taken during epochs 1 and 2. Maps involving (not involving) "cg" means heliospheric frame (spacecraft frame). In the first four subdirectories, file names are of the forms ha60.hide-trp-flux100-hi-N-flux.ext and ha60.hide-trp-mono_80-P.PP-flux.ext, where "ext" is "png" or "txt" according to which product is requested, N is the energy step number for the IBEX-Hi instrument (2-6), P.PP is the energy level, in keV, of a monoenergetic flux. Files in the "combined" subdirectories are named "combined-P.PP-flux.ext, where P.PP has the same meaning as above. In addition to the flux maps to which VEPO provides access, several map files whose data support the determination of the fluxes are also available in the underlying nssdcftp directories and are described by aareadme files there (and by IBEX web pages at SWRI: http://ibex.swri.edu/ibexpublicdata/Data_Release_2/)

18) IBEX-Lo Angular Histograms maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/Angular_Histograms
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Lo Resource:NumericalData
Each table (CSV file) captures the numbers of counts of arriving energetic neutral atoms, as integrated over a full 8-day orbit, for a single IBEX-Lo energy step, for one of two categories of species (hydrogen, oxygen plus carbon, the latter being labelled "Oxygen" in file names). Numbers of counts are given in 360 1-degree bands in spacecraft spin phase. Each table is CSV-formatted Excel. Each subdirectory is for a given energy band and has the tables (files) for each of several orbits for each of the two species categories.

19) IBEX-Lo Direct Events maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/Direct_Events
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Lo Resource:NumericalData
Each record captures the characteristics of one energetic neutral atom arriving at IBEX-Lo. Included is a time tag (seconds since 00:00 UT of January 6, 1980), an arrival direction (R.A. and Dec. in J2000 celestial coordinates), the IBEX location, ENA energy band, species (hydrogen or oxygen) and coincidence type. Data files are given for each 8-day orbit and for each of the 8 IBEX-Lo energy bands. The data files are in ASCII.

20) IBEX-Lo Histograms maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/Histograms
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Lo Resource:NumericalData
Each record captures the number of arriving ENA's of a specific energy band, coincidence type, species (hydrogen or oxygen) and spin phase. Data for each full ~15s spacecraft spin are given at each of 60 spin phases in sequential records, with the J2000 right ascension and declination for look directions corresponding to each spin phase being given in the corresponding record. Also included in each record are a time tag (seconds since 00:00 UT of January 6, 1980), the IBEX location, ENA energy band, species and coincidence type. Data files are given for each 8-day orbit and for each of the 8 IBEX-Lo energy bands. The data files are in ASCII.

21) IBEX-Lo maps in PNG display format every 6 months maxmize
Resource ID:spase://VEPO/DisplayData/IBEX/Lo/Maps-PNG
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Lo Resource:DisplayData
Hydrogen ENA fluxes in each of three IBEX-Lo energy bands in each of 21,600 [720(longitude) by 30(latitude)] bins, accumulated over 6 months. Bins are defined in J2000 ecliptic coordinates. Maps are available for energy bands 5 (209 eV), 6 (439 eV), and 7 (872 eV). PNG-formatted image files are 24 KB in size. Digital versions of these images in txt format are identified by VEPO as a separate data product.

22) IBEX-Lo digital maps every 6 months maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/Maps-TXT
Start:2008-12-10 00:00:00 Observatory:IBEX Cadence:6 months
Stop:2009-06-19 00:00:00 Instrument:IBEX-Lo Resource:NumericalData
Hydrogen ENA fluxes in each of three IBEX-Lo energy bands in each of 21,600 [720(longitude) by 30(latitude)] bins, accumulated over 6 months. Bins are defined in J2000 ecliptic coordinates. Maps are available for energy bands 5 (209 eV), 6 (439 eV), and 7 (872 eV). Digital image files are between 290 and 310 KB in size. Images in PNG format are identified by VEPO as a separate data product.

23) IBEX-Lo Release-3 Counts for flow latitude analysis maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/Release_3/Angular
Start:2009-01-09 15:58:00 Observatory:IBEX Cadence:8 days
Stop:2010-01-09 15:58:00 Instrument:IBEX-Lo Resource:NumericalData
This product contains counts accumulated in each of 30 6-deg spin phase bins over some variable time span indicated in each record. The time spans are selected to support analysis of the flow latitude of the interstellar medium (ISM). The data are specifically as used in the analyses reported in Bzowski et al (2012) and Mobius et al (2012). A companion product has the counting data used in the ISM flow longitude analyses of the same papers. Data are organized into orbit-specific arrays wherein the columns contain the counts for a given time span within the orbit and the rows contain the counts for a given one of the 30 spin-phase angles for the multiple time spans of the orbit. Arrays are available for orbits 12-19, 60, 61, and 63-67. The number of time spans used in an orbit varies from 5 to 38.

24) IBEX-Lo Release-3 Counts for flow longitude analysis maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/Release_3/Counts
Start:2009-01-09 15:58:00 Observatory:IBEX Cadence:8 days
Stop:2010-01-09 15:58:00 Instrument:IBEX-Lo Resource:NumericalData
This product contains counts accumulated in each of 30 6-deg spin phase bins over some variable time span indicated in each record. The time spans are selected to support analysis of the flow longitude of the interstellar medium (ISM). The data are specifically as used in the analyses reported in Bzowski et al (2012) and Mobius et al (2012). A companion product has the counting data used in the ISM flow latitude analyses of the same papers. Data are organized into orbit-specific arrays wherein the columns contain the counts for a given time span within the orbit and the rows contain the counts for a given one of the 30 spin-phase angles for the multiple time spans of the orbit. Arrays are available for orbits 12-19, 60, 61, and 63-67. The number of time spans used in an orbit varies from 5 to 45.

25) IBEX-Lo TOF Histograms maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/Lo/TOF_Histograms
Start:2008-12-25 00:00:00 Observatory:IBEX Cadence:6 minutes
Stop:2009-06-19 00:00:00 Instrument:IBEX-Lo Resource:NumericalData
Each table (CSV file) captures the numbers of counts of arriving energetic neutral atoms, as integrated over a full 8-day orbit, for a single IBEX-Lo energy step, for one of three categories of species (hydrogen, oxygen plus carbon, and hydrogen plus oxygen plus carbon, the latter two being labelled "Oxygen" and "All," respectively in file names). Numbers of counts are given in 1024 0.33-nanosecond TOF bins ranging from 0-0.33 ns to 339.67-340 ns. Each table is CSV-formatted Excel. Each subdirectory is for a given energy band and has the tables (files) for each of several orbits for each of the three species categories.

26) IMAGE EUV Key Parameters: Ion Images maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/EUV/PT600S
Start:2000-03-28 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:Extreme Ultraviolet Imager (EUV) Resource:DisplayData
IMAGE EUV Key Parameters, Ion Images, 10-min resolution

27) IMAGE FUV Substorm Onset Catalog maxmize
Resource ID:spase://VSPO/Catalog/IMAGE/FUV/CATALOG
Start:2000-05-16 00:00:00 Observatory:IMAGE Cadence:
Stop: Instrument:Far Ultraviolet Imager (FUV) Resource:Catalog
This is a table of times of substorm onsets observed by IMAGE/FUV. The raw instrument counts in the FUV image with the greatest number of counts at time of onset, the X and Y pixel numbers for this greatest-count pixel, the onset geographic and geomagnetic latitude and longitude angles and local time, and the geocentric distance of IMAGE are also given for each onset.

28) IMAGE FUV SI plots of O/N2 Ratios maxmize
Resource ID:spase://VEPO/DisplayData/IMAGE/FUV/SI/O_N2_Ratios
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:2 minutes
Stop:2005-05-18 23:59:59 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
This data set consists of images of thermospheric O/N2 column density ratios at 2-min resolution during times of strong geomagnetic storms (Dst.LT.-80nT) of 2000-2005. The ratios are generated from dayside airglow observations of the IMAGE Far Ultraviolet (FUV) Spectrographic Imager (SI). The SI has a peak response at the OI 135.6 nm oxygen emission line and a bandpass of 131.0 to 140.0 nm which includes the LBH band from N2 molecules. For each O/N2 plot, there is a plot of the SI image from which the O/N2 plot was generated, and there is an IDL saveset of the content of the O/N2 maps. The Information URL of this descriptor identifies detailed discussions of the derivations of O/N2 rations from the SI images.

29) IMAGE FUV SI plots of O/N2 Ratios maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/SI/O_N2_Ratios
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:2 minutes
Stop:2005-05-18 23:59:59 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
This data set consists of images of thermospheric O/N2 column density ratios at 2-min resolution during times of strong geomagnetic storms (Dst.LT.-80nT) of 2000-2005. The ratios are generated from dayside airglow observations of the IMAGE Far Ultraviolet (FUV) Spectrographic Imager (SI). The SI has a peak response at the OI 135.6 nm oxygen emission line and a bandpass of 131.0 to 140.0 nm which includes the LBH band from N2 molecules. For each O/N2 plot, there is a plot of the SI image from which the O/N2 plot was generated, and there is an IDL saveset of the content of the O/N2 maps. The Information URL of this descriptor identifies detailed discussions of the derivations of O/N2 rations from the SI images.

30) IMAGE FUV SIE Auroral Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/SIE/PT124S
Start:2000-04-25 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Electron Auroral Images at 1356A, Key Parameters, IMAGE Far UltraViolet (FUV) Spectrographic Imaging camera Electrons (SIE)

31) IMAGE FUV SIP Auroral Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/SIP/PT124S
Start:2000-04-25 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Proton Auroral Images at 1218A, Key Parameters, IMAGE Far UltraViolet (FUV) Spectrographic Imaging camera Protons (SIP)

32) IMAGE FUV WIC Auroral Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/WIC/PT124S
Start:2000-04-25 00:00:00 Observatory:IMAGE Cadence:
Stop:2016-09-14 07:59:48 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Auroral Images, Key Parameters, IMAGE Far UltraViolet (FUV) Wide-band Imaging Camera (WIC)

33) IMAGE FUV/WIC Auroral Images maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/WIC/PT6M
Start:2000-05-19 00:00:00 Observatory:IMAGE Cadence:6 minutes
Stop:2000-12-18 00:00:00 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Auroral Images in GIF format from the Wideband Imaging Camera (WIC) of the Far Ultraviolet (FUV) experiment on IMAGE, at UCB

34) IMAGE HENA Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/HENA/124S
Start:2000-04-21 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:High-Energy Neutral Atom Imager (HENA) Resource:DisplayData
IMAGE High Energy Neutral Atom (HENA) images for several energy channels <10 to 60 keV, key parameters,

35) IMAGE housekeeping data in UDF, all instruments maxmize
Resource ID:spase://VSPO/NumericalData/IMAGE/HK/UDF/Data
Start:2000-05-01 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 23:59:59 Instrument:Low-Energy Neutral Atom Imager (LENA) Resource:NumericalData
This is a set of data at multiple processing levels from all IMAGE instruments. Built by a UNIX-afficionado requiring editing .cshrc's, etc., the data are in Universal Data Format (UDF), and at the moment, has no PC install documentation. UDF software is available to read the IMAGE UDF files.

36) IMAGE LENA Low Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/LENA/PT124S
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 23:59:59 Instrument:Low-Energy Neutral Atom Imager (LENA) Resource:DisplayData
This set of images from IMAGE Low-Energy Neutral Atom (LENA) contains key parameters for several energy channels from 20 to 200 keV.

37) IMAGE MENA Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/MENA/PT124S
Start:2000-04-04 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 23:59:59 Instrument:Medium-Energy Neutral Atom Imager (MENA) Resource:DisplayData
This set of images and movies from IMAGE Medium-Energy Neutral Atom (MENA) contains key parameters for several energy channels from 1 to 70 keV.

38) IRIS Calibrated Images and Spectra Data maxmize
Resource ID:spase://VSPO/NumericalData/IRIS/IRIS/PT1S
Start:2013-09-15 00:00:01 Observatory:Interface Region Imaging Spectrograph (IRIS) Cadence:1 second
Stop:2016-09-14 07:59:51 Instrument:Interface Region Imaging Spectrograph (IRIS) Resource:NumericalData
This data set contains calibrated level-2 images and spectra data from the Interface Region Imaging Spectrograph (IRIS). UV images from IRIS telesccope record observations of features as small as 240 km (150 miles) on the sun every five to ten seconds at specific temperatures, ranging from 5,000 K and 65,000 K (and up to 10 million K during solar flares). This range is tailored to observe material traveling on the surface of the sun, called the photosphere, and in the lowermost layers of the atmosphere, called the chromosphere and transition region. Spectra are obtained every one to two seconds along a slit (1/3 arcsec wide) of solar material at temperatures from 5,000 K to 10 million K, providing information on exactly how much light is visible from any specific wavelength. This corresponds to how much material is present at specific velociites, temperatures and densities. The level-2 data is corrected for dark current, flat-field, and geometric deformation, scaled to the same plate-scale, and packaged into timeseries of slitjaw images and spectral raster scans. The calibration is preliminary and will improve in the coming months.

39) JSPO Solar Image Data maxmize
Resource ID:spase://VSPO/NumericalData/JSPO/MOTH/PT3600.00S
Start:2003-01-01 00:00:00 Observatory:JSPO Cadence:3600.00 seconds
Stop:2003-01-20 00:00:00 Instrument:MOTH Magneto Optical filters at Two Heights Resource:NumericalData
Jeffreys South Pole Observatory (JSPO) solar intensity and LOS_velocity data at 5890A and 7699A

40) KSO Ca II K Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/KSO/KANZ/CaIIK
Start:2010-07-31 00:00:00 Observatory:KSO Cadence:
Stop:2016-09-14 07:59:48 Instrument:KANZ (VSO notation) Resource:NumericalData
Ca II K solar imagery from Kanzelhoehe Solar Observatory (KSO), Austria

41) KSO H-alpha Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/KSO/KANZ/H-alpha
Start:2000-01-20 00:00:00 Observatory:KSO Cadence:
Stop:2016-09-14 07:59:48 Instrument:KANZ (VSO notation) Resource:NumericalData
H-alpha solar imagery from Kanzelhoehe Solar Observatory (KSO), Austria

42) KSO Whitelight Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/KSO/KANZ/Whitelight
Start:2007-07-02 00:00:00 Observatory:KSO Cadence:
Stop:2016-09-14 07:59:48 Instrument:KANZ (VSO notation) Resource:NumericalData
Whitelight solar imagery from Kanzelhoehe Solar Observatory (KSO), Austria

43) NSO/KP Coronal Hole Maps maxmize
Resource ID:spase://VSPO/DisplayData/KittPeak/VacuumTelescope/P27D
Start:1989-09-12 00:00:00 Observatory:Kitt Peak Cadence:27 days
Stop:2002-03-30 00:00:00 Instrument:Kitt Peak Vacuum Telescope (KPVT) Resource:DisplayData
These are PDF files organized as one plot (one file) per 27.27 day Carrington rotation. The files are determined from 1083 nm He I observations made at Kitt Peak.

44) OAC H-alpha Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/OAC/OACT/H-ALPHA
Start:2002-02-26 00:00:00 Observatory:OAC Cadence:
Stop:2016-09-14 07:59:49 Instrument:OACT (VSO notation) Resource:DisplayData
H-alpha solar imagery from Osservatorio Astrofisica di Catania (OAC), Sicily, Italy

45) OBSPM H-alpha Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/OBSPM/H-ALPHA
Start:2004-10-22 00:00:00 Observatory:OBSPM Cadence:
Stop:2016-09-14 07:59:49 Instrument:OBSPM Heliograph Resource:DisplayData
H-alpha solar imagery from OBservatoire Solaire de Paris a Meudon (OBSPM)

46) PICARD SODISM Level 1 Data maxmize
Resource ID:spase://SMWG/NumericalData/PICARD/SODISM/Level1/PT1M
Start:2010-07-01 00:00:00 Observatory:PICARD Cadence:1 minute
Stop:2013-03-31 23:59:00 Instrument:SOlar Diameter Imager and Surface Mapper (SODISM) Resource:NumericalData
Solar images are available from the SOlar Diameter Imager and Surface Mapper (SODISM) onboard the Picard space mission from the middle ultraviolet to the near infrared in five narrow spectral bands centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. Various products are available, including limb image for helioseismology (HL), macros pixel image for helioseismology (HMP), dark current - full image (CO), dark current - limb image (LCO), limb image for diameter (DL), solar rotation full image (RS), and stellar calibration (ES).

47) Polar PIXIE Auroral X-ray Plots and Movies, CDAWeb maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/PIXIE/CDAWEB
Start:1996-03-19 00:00:00 Observatory:POLAR Cadence:
Stop:2002-11-09 00:00:00 Instrument:Polar Ionospheric X-ray Imaging Experiment (PIXIE) Resource:DisplayData
Polar PIXIE Auroral X-Ray Plots and Movies, CDAWeb

48) Polar PIXIE Auroral X-ray Plots and Movies maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/PIXIE/PT10M
Start:1996-03-19 00:00:00 Observatory:POLAR Cadence:10 minutes
Stop:2002-11-09 00:00:00 Instrument:Polar Ionospheric X-ray Imaging Experiment (PIXIE) Resource:DisplayData
Polar PIXIE Auroral X-Ray Plots and Movies

49) Polar PIXIE Level 1 Data Archive maxmize
Resource ID:spase://VSPO/NumericalData/POLAR/PIXIE/PT60.00S
Start:1996-03-15 00:00:00 Observatory:POLAR Cadence:60.00 seconds
Stop:2003-12-29 00:00:00 Instrument:Polar Ionospheric X-ray Imaging Experiment (PIXIE) Resource:NumericalData
Polar PIXIE Level 1 Auroral X-ray Data Archive in CDF Format

50) Polar Ultraviolet Imager H0 High-Resolution Images maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/UVI/H0
Start:1996-03-23 15:56:15 Observatory:POLAR Cadence:
Stop:2008-02-10 18:40:28 Instrument:Ultraviolet Imager (UVI) Resource:DisplayData
This data set contains detected and produced images of the ultraviolet light of the aurora, day and night. from the Polar UltraViolet Imager (UVI) experiment.

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